Hubble observed this galaxy as part of a study for a dataset about close-by AGNs, which will function as a resource for astronomers investigating AGN physics, black holes, host galaxy structure, and more.
An astronaut aboard the area shuttle bus Atlantis captured this image of the Hubble Space Telescope on May 19, 2009. Credit: NASA.
Lenticular galaxies are a special class of galaxies that show functions of both spiral and elliptical galaxies. These intermediate-type galaxies have a flattened disk-like structure, similar to spiral galaxies, however do not have the unique spiral arms.
Seyfert galaxies are a subclass of active galaxies that possess active stellar nuclei (AGNs) at their. Seyfert galaxies stand out from other AGN-containing galaxies because their host galaxy structures remain plainly noticeable, in spite of the extreme radiation discharged by the AGN.
The Hubble Space Telescope is a big, space-based observatory released into orbit by NASA in 1990. Positioned above Earths atmosphere, Hubble is free from atmospheric distortions and has the capability to capture exceptionally detailed and clear images of celestial objects. The telescope has actually played an essential role in advancing our understanding of the universe, contributing to many discoveries and advancements in astrophysics, such as the expansion rate of deep space, the age of deep space, and the existence of dark energy.
The Hubble Space Telescope has actually caught this image of the lenticular galaxy NGC 5283, which contains an active galactic nucleus (AGN) at its core. Home to a supermassive great void, the AGN gives off light across the electro-magnetic spectrum as dust and gas are attracted and heated up. Unlike other AGNs, NGC 5283 is a Seyfert galaxy, with its structure clearly visible. Hubbles observation of NGC 5283 belongs to a study to develop a dataset on neighboring AGNs, aimed at enhancing research study on AGN physics, great voids, and host galaxy structure. Credit: NASA, ESA, A. Barth (University of California– Irvine), and M. Revalski (STScI); Processing: Gladys Kober (NASA/Catholic University of America).
The Hubble Space Telescope has actually imaged lenticular galaxy NGC 5283, a Seyfert galaxy with a visible structure and an active galactic nucleus. The observation belongs to a dataset study to study AGN physics, great voids, and galaxy structures.
The lenticular galaxy NGC 5283 is the topic of this NASA Hubble Space Telescope image. An AGN is a very brilliant region at the heart of a galaxy where a supermassive black hole exists.
NGC 5283 is a Seyfert galaxy. About 10 percent of all galaxies are Seyfert galaxies, and they differ from other galaxies that include AGNs because the galaxy itself is plainly noticeable. Other AGNs release so much radiation that they outperform or make it impossible to observe the structure of their host galaxy!
About 10 percent of all galaxies are Seyfert galaxies, and they vary from other galaxies that contain AGNs due to the fact that the galaxy itself is clearly visible. Lenticular galaxies are a distinct class of galaxies that exhibit functions of both spiral and elliptical galaxies. These intermediate-type galaxies have actually a flattened disk-like structure, comparable to spiral galaxies, however lack the distinct spiral arms. Seyfert galaxies are a subclass of active galaxies that have active stellar nuclei (AGNs) at their. Seyfert galaxies stand out from other AGN-containing galaxies because their host galaxy structures stay clearly visible, regardless of the extreme radiation released by the AGN.
